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火星奥西亚平原的一个低反照率、薄且抗性单元:火星外火星车着陆点存在空降沉积物和后期地下水活动的证据。

A Low Albedo, Thin, Resistant Unit in Oxia Planum, Mars: Evidence for an Airfall Deposit and Late-Stage Groundwater Activity at the ExoMars Rover Landing Site.

作者信息

Harris E, Davis J M, Grindrod P M, Fawdon P, Roberts A L

机构信息

Department of Science Natural History Museum London UK.

Department of Earth Science and Engineering Imperial College London London UK.

出版信息

J Geophys Res Planets. 2024 Nov;129(11):e2024JE008527. doi: 10.1029/2024JE008527. Epub 2024 Nov 22.

Abstract

Oxia Planum, Mars, is the future landing site of the ExoMars rover mission, which will search for preserved biosignatures in a phyllosilicate-bearing unit. Overlying the mission-important phyllosilicate-bearing rocks is a dark, capping unit-known here as the Low albedo, Thin, Resistant (LTR) unit-which may have protected the phyllosilicate-bearing unit over geologic time from solar insolation and radiation. However, little is known about the origin of the LTR unit. Here, we map the LTR unit and investigate its distribution and morphology across 50,000 km using a variety of orbital remote sensing data sets. The characteristics of the LTR unit include draping palaeo-topographic surfaces, deposition over a wide elevation range, and a consistent vertical thickness that can be best explained by airfall deposition including a primary or reworked volcanic palaeo-ashfall. Previous research suggests that the LTR unit was not significantly buried, and we find it to be preferentially preserved with a high mechanical strength in discrete deposits representing palaeo-topographic lows. We suggest this could be attributed to localized cementation via upwelling groundwater. This scenario suggests that most of the phyllosilicate-bearing exposures may not have been protected over geologic time, as the uncemented LTR sediment would have easily been removed by erosion. However, our observations indicate that the scarped margins of the LTR unit deposits probably exposed regions of the once protected phyllosilicate-bearing unit. These areas could be key science targets for the ExoMars rover mission.

摘要

火星的奥克西亚平原是“火星外天体生物学探测器”任务的未来着陆点,该任务将在一个含页硅酸盐的单元中寻找保存下来的生物特征。覆盖在对该任务至关重要的含页硅酸盐岩石之上的是一个深色的覆盖单元,这里称为低反照率、薄层、抗性(LTR)单元,它可能在地质时期保护了含页硅酸盐单元免受日照和辐射。然而,人们对LTR单元的起源知之甚少。在这里,我们绘制了LTR单元的地图,并使用各种轨道遥感数据集研究了其在50000平方千米范围内的分布和形态。LTR单元的特征包括覆盖古地形表面、在很宽的海拔范围内沉积以及一致的垂直厚度,这最好用包括原生或再加工的火山古灰降在内的空降沉积来解释。先前的研究表明,LTR单元没有被大量掩埋,我们发现它在代表古地形低洼的离散沉积物中以高机械强度优先保存下来。我们认为这可能归因于上升的地下水导致的局部胶结作用。这种情况表明,大部分含页硅酸盐的露头在地质时期可能没有受到保护,因为未胶结的LTR沉积物很容易被侵蚀掉。然而,我们的观察表明,LTR单元沉积物陡峭的边缘可能暴露了曾经受保护的含页硅酸盐单元的区域。这些区域可能是“火星外天体生物学探测器”任务的关键科学目标。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/114a/11583114/4810e2e8bff0/JGRE-129-0-g004.jpg

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